The inferred \(L_{\text{\,acc}}\)  values found in the Hei differ slightly from those of the Hi lines. This is likely due to the complexity of processes that the Hei lines are tracing, which include accretion, but not exclusively. In particular there can be a strong wind emission [1]}, [2]}, [3]}. Therefore we have decided to estimate \(L_{\text{\,acc}}\)  using the Hi emission lines only.
